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Table 2:

Unresolved sources which are denoted in Figs. 4-7. The error of the flux densities was calculated assuming a 5% calibration error.
No. RA Dec $S_{\lambda90}~{\rm [mJy]}$ $S_{\lambda20}~{\rm [mJy]}$ $S_{\lambda6.2}~{\rm [mJy]}$ $S_{\lambda3.6}~{\rm [mJy]}$ $\alpha $
1 $00^{\rm h} 47^{\rm m} 00\hbox{$.\!\!^{\rm s}$ }02$ $-25^\circ 23' 50\hbox{$.\!\!^{\prime\prime}$ }1$   $4.1\pm 0.2$ $2.2\pm 0.1$   $0.5\pm0.2$
2 $00^{\rm h} 47^{\rm m} 12\hbox{$.\!\!^{\rm s}$ }01$ $-25^\circ 17' 43\hbox{$.\!\!^{\prime\prime}$ }9$   $17.3\pm 1.0$ $6.6\pm 0.3$   $0.8\pm0.2$
3 $00^{\rm h} 47^{\rm m} 33\hbox{$.\!\!^{\rm s}$ }12$ $-25^\circ 17' 17\hbox{$.\!\!^{\prime\prime}$ }3$ $3960\pm 80$ $2040\pm 100$ $1270\pm 60$ $980\pm 50$ $0.44\pm0.02$
4 $00^{\rm h} 47^{\rm m} 44\hbox{$.\!\!^{\rm s}$ }91$ $-25^\circ
13' 38\hbox{$.\!\!^{\prime\prime}$ }4$   $26\pm 2$ $7.9\pm 0.4$   $1.0\pm0.2$
5 $00^{\rm h} 47^{\rm m} 52\hbox{$.\!\!^{\rm s}$ }41$ $-25^\circ
15' 44\hbox{$.\!\!^{\prime\prime}$ }8$     $1.5\pm 0.2$    
6 $00^{\rm h} 47^{\rm m} 58\hbox{$.\!\!^{\rm s}$ }90$ $-25^\circ 18' 31\hbox{$.\!\!^{\prime\prime}$ }9$ $190\pm 10$ $53\pm 3$ $19\pm 1$ $9.5\pm 0.5$ $0.84\pm0.02$
7 $00^{\rm h} 48^{\rm m} 00\hbox{$.\!\!^{\rm s}$ }84$ $-25^\circ 16' 26\hbox{$.\!\!^{\prime\prime}$ }3$   $2.1\pm 0.3$ $1.10\pm 0.06$   $0.5\pm0.2$
8 $00^{\rm h} 48^{\rm m} 05\hbox{$.\!\!^{\rm s}$ }0$ $-25^\circ 11' 11\hbox{$.\!\!^{\prime\prime}$ }8$   $5.3\pm 0.3$ $3.05\pm 0.15$   $0.4\pm0.2$

Source LaTeX | All tables | In the text

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